CSIRO has a cold spray research group which is developing cold sprayed Invar. This project will be developing an optical metrology setup to measure the creep of the cold sprayed Invar in collaboration with CSIRO Lab22 in Clayton, Victoria.

This project aims to address the potential of Spatial Light Modulators (SLMs) as highly nonlinear optical elements, including their potential use in pyramid wavefront sensing.

This project aims to address the potential of Spatial Light Modulators (SLMs) as highly nonlinear optical elements, including their potential use in pyramid wavefront sensing.

Using both the Wide-Field Spectrograph (WiFeS) on the ANU 2.3m telescope and the 1.4 GHz radio band on the Australia Telescope Compact Array (ATCA), the student will address how the radio jets from the supermassive black hole interact with the Seyfert host galaxy to affect the evolution of the galaxy.

Accreted stellar populations are comprised of the remnants of destroyed galaxies, and often dominate the 'stellar haloes' of galaxies such as the Milky Way.

The successful applicant will join the ANU team and will assist with the development of instrumentation for the optical communication team

The successful applicant will join the ANU team and will assist with the development of instrumentation for the optical communication team

This project aims to utilize LLMs (Large Language Models) to enhance the usability of systems engineering documentation, including system requirement documents and flowdowns, interface documents, design documents, and reliability assessments.

This project aims to utilize LLMs (Large Language Models) to enhance the usability of systems engineering documentation, including system requirement documents and flowdowns, interface documents, design documents, and reliability assessments.

This project aims to utilize LLMs (Large Language Models) to enhance the usability of systems engineering documentation, including system requirement documents and flowdowns, interface documents, design documents, and reliability assessments.

This project requires significant data analysis efforts and some observational and theoretical efforts.

With this project we will be using the newly automated ANU 2.3m telescope and the powerful WiFeS optical spectrograph to perform a time-series measurement of luminous active galaxies (AGN) using the technique of Quasar Reverberation Mapping.

A student undertaking this project will investigate the potential customisations of lenslet arrays afforded by optical meta-surfaces, and propose designs to be fabricated in the Research School of Physics at ANU.

A student undertaking this project will investigate the potential customisations of lenslet arrays afforded by optical meta-surfaces, and propose designs to be fabricated in the Research School of Physics at ANU.

A student undertaking this project will investigate the potential customisations of lenslet arrays afforded by optical meta-surfaces, and propose designs to be fabricated in the Research School of Physics at ANU.